To study the dynamical evolution of dense nuclear matter, the model has been implemented in the hadronic transport code SMASH [1]} through solving the relativistic mean-field equations of motion derived from the VDF EOS (Sec. ). For investigating the qualitative features of the behavior of dense nuclear matter, we have concentrated on one specific realization of the dense matter EOS, keeping in mind that the ultimate motivation behind creating the VDF model and its supporting framework within SMASH is to enable large-scale comparisons between experimental data and simulations spanning a broad family of EOSs.
